NGC 7316 is a barred spiral galaxy in the constellation of Pegasus. Its velocity with respect to the cosmic microwave background is 5,198±25 km/s, which corresponds to a Hubble distance of 250.1 ± 17.5 Mly (76.67 ± 5.38 Mpc). However, three non-redshift measurements give a closer mean distance of 212.87 ± 3.89 Mly (65.267 ± 1.192 Mpc). It was discovered by German-British astronomer William Herschel on 18 September 1784. NGC 7316 has a possible active galactic nucleus, i.e. it has a compact region at the center of a galaxy that emits a significant amount of energy across the electromagnetic spectrum, with characteristics indicating that this luminosity is not produced by the stars. NGC 7316 is also a starburst galaxy. NGC 7316 has a nucleus with excessive amounts of ultraviolet emissions compared with other galaxies, and is listed in the Markarian catalogue as MRK 307.
Galaxy group According to M. J. Geller and J. P. Huchra, NGC 7316 is a member of a galaxy group which contains 2 other galaxies: NGC 7321 and NGC 7323.
Supernovae Two supernovae have been observed in NGC 7316:
SN 2006cx (Type II, mag. 17.4) was discovered by the Lick Observatory Supernova Search (LOSS) on 8 June 2006. SN 2016hvu (Type II-P, mag. 17.6) was discovered by the Catalina Real-time Transient Survey on 6 November 2016.
See also List of NGC objects (7001–7840)
References
External links Media related to NGC 7316 at Wikimedia Commons NGC 7316 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


